×

Acceleration of particles by black hole with gravitomagnetic charge immersed in magnetic field. (English) Zbl 1286.83048

Summary: The collision of test charged particles in the vicinity of an event horizon of a weakly magnetized non-rotating black hole with gravitomagnetic charge has been studied. The presence of the external magnetic field decreases the innermost stable circular orbits (ISCO) radii of charged particles. The opposite mechanism occurs when there is nonvanishing gravitomagnetic charge. For a collision of charged particle moving at ISCO and the neutral particle falling from infinity the maximal collision energy can be decreased by gravitomagnetic charge in the presence of external asymptotically uniform magnetic field.

MSC:

83C57 Black holes
83C10 Equations of motion in general relativity and gravitational theory
78A35 Motion of charged particles

References:

[1] Abdujabbarov, A.A., Ahmedov, B.J., Kagramanova, V.G.: Gen. Relativ. Gravit. 40, 2515 (2008) · Zbl 1162.83306 · doi:10.1007/s10714-008-0635-3
[2] Abdujabbarov, A.A., Ahmedov, B.J., Shaymatov, S.R., Rakhmatov, A.S.: Astrophys. Space Sci. 334, 237 (2011) · Zbl 1230.83053 · doi:10.1007/s10509-011-0740-8
[3] Ahmedov, B.J., Rakhmatov, N.I.: Found. Phys. 33, 625 (2003) · doi:10.1023/A:1023722704270
[4] Ahmedov, B.J., Khugaev, A.V., Abdujabbarov, A.A.: Astrophys. Space Sci. 337, 679 (2012) · doi:10.1007/s10509-011-0862-z
[5] Aliev, A.N.: Phys. Rev. D 77, 044038 (2008)
[6] Aliev, A.N., Cebeci, H., Dereli, T.: Phys. Rev. D 77, 124022 (2008)
[7] Banados, M., Silk, J., West, S.M.: Phys. Rev. Lett. 103, 111102 (2009) · doi:10.1103/PhysRevLett.103.111102
[8] Berti, E., Cardoso, V., Gualtieri, L., Pretorius, F., Sperhake, U.: Phys. Rev. Lett. 103, 239001 (2009) · doi:10.1103/PhysRevLett.103.239001
[9] Bini, D., Cherubini, C., Janzen, R.T., Mashhoon, B.: Class. Quantum Gravity 20, 457 (2003) · Zbl 1047.83006 · doi:10.1088/0264-9381/20/3/305
[10] Chowdhury, A.N., Patil, M., Malafarina, D., Joshi, P.S.: Phys. Rev. D 85, 104031 (2012) · doi:10.1103/PhysRevD.85.104031
[11] Dadhich, N., Turakulov, Y.Z., Class. Quantum Gravity 20, 457 (2003) · Zbl 1047.83006 · doi:10.1088/0264-9381/20/3/305
[12] Frolov, V.P.: Phys. Rev. D 85, 024020 (2012)
[13] Kagramanova, V., Kunz, J., Lämmerzahl, C.: Class. Quantum Gravity 25, 105023 (2008) · Zbl 1140.83324 · doi:10.1088/0264-9381/25/10/105023
[14] Kagramanova, V., Kunz, J., Hackmann, E., Lammerzahl, C.: Phys. Rev. D 81, 124044 (2010) · doi:10.1103/PhysRevD.81.124044
[15] Lynden-Bell, D., Nouri-Zonoz, M.: Rev. Mod. Phys. 70, 427 (1998) · Zbl 1205.83054 · doi:10.1103/RevModPhys.70.427
[16] Morozova, V.S., Ahmedov, B.J.: Int. J. Mod. Phys. D 18, 107 (2009) · Zbl 1163.83342 · doi:10.1142/S0218271809014352
[17] Morozova, V.S., Ahmedov, B.J., Kagramanova, V.G.: Astrophys. J. 684, 1359 (2008) · doi:10.1086/590322
[18] Newman, E., Tamburino, L., Unti, T.: J. Math. Phys. 4, 915 (1963) · Zbl 0115.43305 · doi:10.1063/1.1704018
[19] Nouri-Zonoz, M.: Class. Quantum Gravity 21, 471 (2004) · Zbl 1045.83026 · doi:10.1088/0264-9381/21/2/011
[20] Nouri-Zonoz, M., Dadhich, N., Lynden-Bell, D.: Class. Quantum Gravity 16, 1021 (1999) · Zbl 0938.83002 · doi:10.1088/0264-9381/16/3/028
[21] Nouri-Zonoz, M., Lynden-Bell, D.: Mon. Not. R. Astron. Soc. 292, 714 (1997) · doi:10.1093/mnras/292.3.714
[22] Patil, M., Joshi, P.S.: Phys. Rev. D 85, 104014 (2012) · doi:10.1103/PhysRevD.85.104014
[23] Penrose, R.: Riv. Nuovo Cimento 1, 252 (1969)
[24] Piran, T., Shaham, J.: Phys. Rev. D 16, 1615 (1977a) · doi:10.1103/PhysRevD.16.1615
[25] Piran, T., Shaham: J. Astrophys. Astron. 214, 268 (1977b)
[26] Piran, T., Katz, J., Shaham, J.: Astrophys. J. Lett. 196, L107 (1975) · doi:10.1086/181755
[27] Piotrovich, M. Y., Silantev, N. A, Gnedin, Y.N., Natsvlishvili, T.M.: Astrophys. Bull. 66, 320 (2011) · doi:10.1134/S1990341311030047
[28] Rahvar, S., Habibi, F.: Astrophys. J. 610, 673 (2004) · doi:10.1086/421728
[29] Zimmerman, R.L., Shahir, B.Y.: Gen. Relativ. Gravit. 21, 821 (1989) · Zbl 0669.53061 · doi:10.1007/BF00758986
This reference list is based on information provided by the publisher or from digital mathematics libraries. Its items are heuristically matched to zbMATH identifiers and may contain data conversion errors. In some cases that data have been complemented/enhanced by data from zbMATH Open. This attempts to reflect the references listed in the original paper as accurately as possible without claiming completeness or a perfect matching.